Comprehensive asymmetric dark matter model
Stephen J. Lonsdale, Raymond R. Volkas

TL;DR
This paper develops a comprehensive asymmetric dark matter model based on mirror matter and asymmetric symmetry breaking, explaining the mass density similarity and linking dark matter mass to the proton mass.
Contribution
It introduces a novel ADM model with spontaneous mirror symmetry breaking and a detailed thermal history, addressing phenomenological and cosmological constraints.
Findings
Dark matter composed of dark neutrons or dark hydrogen atoms.
Dark sector electroweak scale larger than visible sector.
Mechanism for lepton asymmetry generation via heavy neutrino decays.
Abstract
Asymmetric dark matter (ADM) is motivated by the similar cosmological mass densities measured for ordinary and dark matter. We present a comprehensive theory for ADM that addresses the mass density similarity, going beyond the usual ADM explanations of similar number densities. It features an explicit matter-antimatter asymmetry generation mechanism, has one fully worked out thermal history and suggestions for other possibilities, and meets all phenomenological, cosmological and astrophysical constraints. Importantly, it incorporates a deep reason for why the dark matter mass scale is related to the proton mass, a key consideration in ADM models. Our starting point is the idea of mirror matter, which offers an explanation for dark matter by duplicating the standard model with a dark sector related by a parity symmetry. However, the dark sector need not manifest as a symmetric copy…
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